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Communication Dans Un Congrès Classical and Quantum Gravity Année : 2010

Noise from scattered light in Virgo's second science run data

T Accadia (1, 2) , F Acernese (1, 3) , F Antonucci (1, 3) , P Astone (1, 3) , G Ballardin (1, 4) , F Barone (1, 3) , M. Barsuglia (1, 5) , Th S Bauer (1, 6) , M G Beker (1, 6) , A Belletoile (1, 2) , S Birindelli (1, 7) , M Bitossi (1, 8) , M A Bizouard (1, 9) , M Blom (1, 6) , François Bondu (10) , L Bonelli (1, 8) , R Bonnand (1) , V Boschi (1, 8) , L Bosi (1, 3) , B Bouhou (1, 5) , S Braccini (1, 8) , C Bradaschia (1, 8) , A Brillet (1, 7) , V Brisson (1, 9) , R Budzyski (1) , T Bulik (1) , H J Bulten (1, 6) , D Buskulic (1, 2) , Christelle Lesvigne-Buy (1, 5) , G Cagnoli (1, 3) , E Calloni (1, 3) , E Campagna (1, 3) , B Canuel (1, 4) , F Carbognani (1, 4) , F Cavalier (1, 9) , R Cavalieri (1, 4) , G Cella (1, 8) , E Cesarini (1, 3) , E Chassande-Mottin (1, 5) , A Chincarini (1, 3) , F Cleva (1, 7) , E Coccia (1, 11) , C N Colacino (1, 8) , J Colas (1, 4) , A Colla (1, 3) , M Colombini (1, 3) , A Corsi (1, 3) , J.-P Coulon (1, 7) , E Cuoco (1, 4) , Antonio 9a (1, 11) , V Dattilo (1, 4) , M Davier (1, 9) , R Day (1, 4) , Rosa 5ab (1, 3) , G Debreczeni (1) , M Del (1) , Prete 7ac (1, 8) , L Di (1) , Fiore 5a (1, 3) , A Di (1) , Lieto 7ab (8) , M Di (1) , Paolo Emilio (1, 11) , Virgilio 7a (8) , A Dietz (1, 2) , M Drago (1, 12, 13) , V Fafone (1, 11) , I Ferrante (1, 8) , F Fidecaro (1, 8) , I Fiori (1, 4) , R Flaminio (1) , J.-D Fournier (1, 7) , J Franc (1) , S Frasca (1, 3) , F Frasconi (1, 8) , A Freise (1, 14) , M Galimberti (1) , L Gammaitoni (1, 3) , F Garufi (1, 3) , M E Gáspár (1) , G Gemme (1, 3) , E Genin (1, 4) , A Gennai (1, 8) , A Giazotto (1, 8) , R Gouaty (1, 2) , M Granata (1, 5) , C Greverie (1, 7) , G M Guidi (1, 3) , J.-F Hayau (10) , H Heitmann (1, 7) , P Hello (1, 9) , S Hild (1, 14) , D Huet (1, 4, 14) , P Jaranowski (1) , I Kowalska (1) , A Królak (1) , N Leroy (1, 9) , N Letendre (1, 2) , T G F Li (6) , M Lorenzini (1, 3) , V Loriette (1, 9) , G Losurdo (1, 3) , E Majorana (1, 3) , I Maksimovic (1, 9) , N Man (1, 7) , M Mantovani (1, 8) , F Marchesoni (1, 3) , F Marion (1, 2) , J Marque (1, 4) , F Martelli (1, 3) , A Masserot (1, 2) , C Michel (1) , L Milano (1, 3) , Y Minenkov (1, 11) , M Mohan (1, 4) , N Morgado (1) , A Morgia (1, 11) , S Mosca (1, 3) , V Moscatelli (1, 3) , B Mours (1, 2) , I Neri (1, 3) , F Nocera (1, 4) , G Pagliaroli (1, 11) , L Palladino (1, 11) , C Palomba (1, 3) , F Paoletti (1, 4, 8) , S Pardi (1, 3) , M Parisi (1, 3) , A Pasqualetti (1, 4) , R Passaquieti (1, 8) , D Passuello (1, 8) , G Persichetti (1, 3) , M Pichot (1, 7) , F Piergiovanni (1, 3) , M Pietka (1) , L Pinard (1) , R Poggiani (1, 8) , M Prato (1, 3) , G A Prodi (1, 12, 13) , M Punturo (1, 3) , P Puppo (1, 3) , D S Rabeling (1, 6) , I Rácz (1) , P Rapagnani (1, 3) , V Re (12, 13) , T Regimbau (1, 7) , F Ricci (1, 3) , F Robinet (1, 9) , A Rocchi (1, 11) , L Rolland (1, 2) , R Romano (1, 3) , D Rosiska (1) , P Ruggi (1, 4) , B Sassolas (1) , D Sentenac (1, 4) , L Sperandio (1, 11) , R Sturani (1, 3) , B L Swinkels (1, 4) , A Toncelli (1, 8) , M Tonelli (1, 8) , O Torre (1, 8) , E Tournefier (1, 2) , F Travasso (1, 3) , G Vajente (1, 8) , J F J van den Brand (1, 6) , S van Der Putten (1, 6) , M Vasuth (1) , M Vavoulidis (1, 9) , G Vedovato (1, 12, 13) , D Verkindt (1, 2) , F Vetrano (1, 3) , A Viceré (1, 3) , J.-y Vinet (1, 7) , H Vocca (1, 3) , M Was (1, 9) , M Yvert (1, 2)
François Bondu
Lieto 7ab
  • Fonction : Auteur
Virgilio 7a
  • Fonction : Auteur

Résumé

Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is back-scattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer.

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Dates et versions

hal-00629992 , version 1 (07-10-2011)

Identifiants

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T Accadia, F Acernese, F Antonucci, P Astone, G Ballardin, et al.. Noise from scattered light in Virgo's second science run data. 14th Gravitational Wave Data Analysis Workshop (GWDAW-14), Jan 2010, rome, Italy. pp.194011, ⟨10.1088/0264-9381/27/19/194011⟩. ⟨hal-00629992⟩
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